V-Band Photometric Monitoring of 782 Montefiore
Abstract
Photometric monitoring of 782 Montefiore was carried out in 2020 February through a Johnson V filter. Based on 247 images collected over three nights, we find a best fit rotation period of 4.073±0.001 h and a V-band variability amplitude of 0.50±0.02 mag, in good agreement with previous results.
- Publication:
-
Minor Planet Bulletin
- Pub Date:
- October 2022
- Bibcode:
- 2022MPBu...49..257B
- Keywords:
-
- Minor Planets;
- Asteroids;
- Light Curves;
- Photometry;
- Periods